TITLE: GCN CIRCULAR NUMBER: 24198 SUBJECT: LIGO/Virgo S190425z: KPED Follow-Up Observations DATE: 19/04/25 21:54:41 GMT FROM: Tomas Ahumada at U. of Maryland Authors: Tomas Ahumada (UMD), Michael W. Coughlin (Caltech), Kai Staats (Embry-Riddle University), Richard G. Dekany (Caltech), Dmitry A. Duev (Caltech), Michael Feeney (Caltech), S. R. Kulkarni (Caltech), Reed Riddle (Caltech) on behalf of the KPED team and the Global Relay of Observatories Watching Transients Happen (GROWTH) collaboration. We used the Kitt Peak EMCCD Demonstrator (KPED) on the Kitt Peak 84-inch telescope (Coughlin et al 2019b) to obtain 300 s r-band images for 10 galaxies in the 90% localization region of the S190425z LIGO/Virgo detection (GCN 24168). The observations started 10:12 UT on 2019 April 25 (about ~1.9 hours after the event) and the median 5 sigma upper limit for an isolated point source in our images was r > 20.8. No transients were detected in any of the galaxies listed below: Name | R.A. | Dec. ------------------------------------------------------------------------ NGC6166 | 16:28:38.23 | 39:33:04.4 NGC4889 | 13:00:08.13 | 27:58:37.2 CB-11.4459 15:18:32.09 | 31:09:40.82 1200-07486009 | 15:12:12.73 | 31:54:36.17 J15122693+3224040 | 15:12:26.92 | 32:24:03.84 J151717.32+304801.3 | 15:17:17.33 | 30:48:01.33 J151303.42+325505.8 | 15:13:03.43 | 32:55:05.81 J15120209+3254551 | 15:12:02.07 | 32:54:55.29 J15113637+3142477 | 15:11:36.34 | 31:42:47.31 J151109.81+313833.2 | 15:11:09.82 | 31:38:33.2 The KPED team thanks the National Science Foundation, the National Optical Astronomical Observatory and the Murty family for support in the building and operation of KPED.